NFW Dark Matter Halos and Virial Radius

In summary, NFW Dark Matter Halos are a density model for the halo developed by Navarro, Frenk, & White (NFW). The density structure is defined by a formula involving the critical density of the universe, the virial radius, and a parameter 200. This 200 value is historically and arbitrarily chosen as the point where the average density of the cluster falls to 200 times the critical density. This definition is not universal, as other papers may use different multipliers such as R500 or R100. The original NFW paper is a good starting point for further research on this topic.
  • #1
zephyr5050
21
0
I've been working with NFW Dark Matter Halos recently. This is a particular density model for the halo developed by Navarro, Frenk, & White (NFW). The density structure has the form
[tex] \rho (r) = \frac{\delta_c \rho_c}{(r/r_s)(1+r/r_s)^2} [/tex]
where
[tex] \delta_c = \frac{200}{3} \frac{c^3}{ln(1+c)-c/(1+c)} [/tex]
[tex] r_s = r_{200}/c [/tex]
and [itex] \rho_c [/itex] is the critical density of the universe (as a function of redshift). The parameter [itex] r_{200} [/itex] is the virial radius which is defined as the radius at which the mass density of the halo is [itex] 200\rho_c [/itex].

Now we can't really talk about the mass of this halo because the integral from 0 to [itex]\infty[/itex] diverges. Instead, we use the fiducial radius [itex]r_{200}[/itex] and define the quantity [itex]M_{200}[/itex] to be the mass inside the radius [itex]r_{200}[/itex]. It can be shown that
[tex] M_{200} = \frac{800\pi}{3}\rho_c r_{200}^3 [/tex]
While all this makes sense to me, there's one thing that I don't understand here. Where does this 200 come from? Why say [itex] r_{200} \equiv 200 \rho_c [/itex]? Is there any logic to this, is it historical, arbitrary? What's going on here?
 
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  • #2
I think it's basically historical and arbitrary. You have to draw a line somewhere, and the accepted way to do it is when the average density of the cluster falls to 200X the critical density. It's not universal, however. You will find papers referring to R500, R100, R150, etc., all defined in the same way, but with different multipliers.
 
  • #3
Do you happen to know the paper which proposed this commonly accepted line? If any?
 
  • #5


I can provide some insight into the reasoning behind using the value of 200 for the virial radius in the NFW dark matter halo model.

The value of 200 comes from the fact that it is a common threshold used to define the virial radius in cosmological simulations and observations. This threshold is based on the assumption that the dark matter halos are in approximate virial equilibrium, meaning that the gravitational forces within the halo are balanced by the kinetic energy of the particles within it.

In other words, the virial radius is the radius at which the average density of the halo is 200 times the critical density of the universe. This value is chosen because it corresponds to the point at which the gravitational potential energy of the halo is equal to its kinetic energy, indicating virial equilibrium.

The use of this threshold is not arbitrary or historical, but rather a practical choice for defining the virial radius in a consistent manner across different simulations and observations. It also allows for a more manageable and meaningful measure of the mass of the halo, as the integral from 0 to infinity diverges when trying to calculate the total mass of the halo.

Overall, the use of 200 for the virial radius in the NFW dark matter halo model is a well-established and widely accepted convention in the field of cosmology.
 

1. What is a NFW dark matter halo?

A NFW (Navarro-Frenk-White) dark matter halo is a theoretical model used to describe the distribution of dark matter in galaxies and galaxy clusters. It is named after the three scientists who developed the model.

2. How is the NFW halo different from other dark matter models?

The NFW halo is different from other dark matter models in that it predicts a specific density profile for dark matter, with the density decreasing as the distance from the center of the halo increases. Other models, such as the isothermal sphere model, have a constant density throughout the halo.

3. What is the virial radius of a dark matter halo?

The virial radius is the distance from the center of the halo at which the average density is equal to the critical density of the universe. It is often used as a measure of the size of the halo.

4. How is the virial radius of a dark matter halo determined?

The virial radius is typically determined by studying the dynamics of galaxies or galaxy clusters within the halo. By measuring the velocities and distances of these objects, scientists can estimate the mass and size of the halo, including the virial radius.

5. What is the significance of the NFW dark matter halo for understanding the structure of the universe?

The NFW dark matter halo is important because it helps explain the observed distribution of matter in the universe. By studying the properties of these halos, scientists can gain insight into the formation and evolution of galaxies and galaxy clusters, as well as the overall structure of the universe.

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